Accretion in the detached post-common-envelope binary LTT 560

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Table 3

Photospheric white dwarf abundances.

Element	log [X/H]_LTT560¹	log [X/H]_⊙²	× solar³

Mg	–6.2	–4.4	0.015
Al	–7.6	–5.6	0.010
Si	–6.2	–4.5	0.018
Ca	–7.5	–5.7	0.015
Sc	–10.9	–8.8	0.008
Mn	–8.2	–6.6	0.018
Fe	–6.3	–4.5	0.018
Co	–8.8	–7.0	0.018
Ni	–7.9	–5.8	0.007

Notes. Abundances determined from fitting TLUSTY/SYNSPEC models to the metal lines detected in the average UVES spectrum of LTT 560.

⁽¹⁾

Metal abundances relative to hydrogen, by number, for LTT 560.

⁽²⁾

As (1), but for the Sun.

⁽³⁾

The abundances in LTT 560 relative to those in the Sun.

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